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Stellar clustering shapes the architecture of planetary systems
Planet formation is generally described in terms of a system containing the host star and a protoplanetary disk(1–3), of which the internal properties (for example, mass and metallicity) determine the properties of the resulting planetary system(4). However, (proto)planetary systems are predicted(5,...
Gespeichert in:
| Veröffentlicht in: | Nature |
|---|---|
| Hauptverfasser: | , , , |
| Format: | Artigo |
| Sprache: | Inglês |
| Veröffentlicht: |
2020
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| Schlagworte: | |
| Online Zugang: | https://ncbi.nlm.nih.gov/pmc/articles/PMC7116760/ https://ncbi.nlm.nih.gov/pubmed/33087913 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1038/s41586-020-2800-0 |
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